Tom Kalbfus
Mongoose
A New Type of Dyson Sphere May Be Nearly Impossible to Detect
Over fifty years ago, physicist Freeman Dyson proposed an awesome, if slightly insane, idea: That an advanced alien civilization might construct a massive, energy-harvesting sphere around its star, and bunk up inside.
Scientists have never given up on Dyson spheres—we've even conducted a few legitimate searches for their infrared heat signatures. Now, physicists Ibrahim Semiz and Salim Ogur may have an explanation for why we can't seem to find the megastructures. If Dyson spheres exist, they're probably a lot smaller than we thought.
Since Dyson first proposed his massive space habitats, scientists have tried to imagine how such structures could physically work. By and large, researchers have focused on Dyson spheres encircling Sun-like stars. But this scenario poses a few major, and perhaps insurmountable, problems. For starters, such a sphere would have to be built at a distance of roughly 1 AU, the same distance between the Earth and the Sun. That means the structure would be utterly massive, requiring huge volumes of material to construct. What's more, the surface of the sphere would experience only minuscule levels of gravity. To live on it, humans would either need substantial genetic modification, or some sort of advanced artificial gravity system, the likes of which we haven't been able to piece together, even theoretically.
From "Relics," the Star Trek episode that introduced millions to Dyson spheres.
A white dwarf star—the dimmer stellar remnant left over after a Sun-like star swells up and explodes—might be a better option for Dyson spheres. A white dwarf's habitable zone is much closer, so the sphere would end up being significantly smaller. The researchers calculate that a one meter-thick sphere built in the habitable zone of a white dwarf would require 10^23 kilograms of matter, slightly less than the mass of our moon. A Dyson sphere encircling a white dwarf would also have almost Earth-like gravity, according to the researchers' calculations.
There's just one catch: Because white dwarfs are less luminous than Sun-like stars, the infrared heat signatures emitted by a white dwarf Dyson sphere would be much smaller and harder to detect. If intelligent aliens are out there, it may be a while yet before our scopes are powerful enough that we're able spot them from Earth. [arXiv via MIT Technology Review]
Top image via Slawek Wojtowicz
A small footnote: The researchers estimate that a Dyson sphere surrounding a white dwarf would be roughly 10 ^6 kilometers in radius. As pointed out by an astute commentator, this puts the newly proposed Dyson sphere within an order of magnitude of the one featured in Star Trek: The Next Generation. It may be new to science, but it seems Star Trek figured this all out loooong ago.
Contact the author at maddie.stone@gizmodo.com or follow her on Twitter.
As an exercise, how big would the Dyson sphere around this star be, and what would be its surface gravity?
Sirius B
With a mass nearly equal to the Sun's, Sirius B is one of the more massive white dwarfs known (0.98 M☉[102]); it is almost double the 0.5–0.6 M☉ average. Yet that same mass is packed into a volume roughly equal to the Earth's.[102] The current surface temperature is 25,200 K.[7] However, because there is no internal heat source, Sirius B will steadily cool as the remaining heat is radiated into space over a period of more than two billion years.[103]
A white dwarf forms only after the star has evolved from the main sequence and then passed through a red-giant stage. This occurred when Sirius B was less than half its current age, around 120 million years ago. The original star had an estimated 5 M☉[7] and was a B-type star (roughly B4–5)[104][105] when it still was on the main sequence. While it passed through the red giant stage, Sirius B may have enriched the metallicity of its companion.
This star is primarily composed of a carbon–oxygen mixture that was generated by helium fusion in the progenitor star.[7] This is overlaid by an envelope of lighter elements, with the materials segregated by mass because of the high surface gravity.[106] Hence the outer atmosphere of Sirius B is now almost pure hydrogen—the element with the lowest mass—and no other elements are seen in its spectrum.[107]

Over fifty years ago, physicist Freeman Dyson proposed an awesome, if slightly insane, idea: That an advanced alien civilization might construct a massive, energy-harvesting sphere around its star, and bunk up inside.
Scientists have never given up on Dyson spheres—we've even conducted a few legitimate searches for their infrared heat signatures. Now, physicists Ibrahim Semiz and Salim Ogur may have an explanation for why we can't seem to find the megastructures. If Dyson spheres exist, they're probably a lot smaller than we thought.
Since Dyson first proposed his massive space habitats, scientists have tried to imagine how such structures could physically work. By and large, researchers have focused on Dyson spheres encircling Sun-like stars. But this scenario poses a few major, and perhaps insurmountable, problems. For starters, such a sphere would have to be built at a distance of roughly 1 AU, the same distance between the Earth and the Sun. That means the structure would be utterly massive, requiring huge volumes of material to construct. What's more, the surface of the sphere would experience only minuscule levels of gravity. To live on it, humans would either need substantial genetic modification, or some sort of advanced artificial gravity system, the likes of which we haven't been able to piece together, even theoretically.

From "Relics," the Star Trek episode that introduced millions to Dyson spheres.
A white dwarf star—the dimmer stellar remnant left over after a Sun-like star swells up and explodes—might be a better option for Dyson spheres. A white dwarf's habitable zone is much closer, so the sphere would end up being significantly smaller. The researchers calculate that a one meter-thick sphere built in the habitable zone of a white dwarf would require 10^23 kilograms of matter, slightly less than the mass of our moon. A Dyson sphere encircling a white dwarf would also have almost Earth-like gravity, according to the researchers' calculations.
There's just one catch: Because white dwarfs are less luminous than Sun-like stars, the infrared heat signatures emitted by a white dwarf Dyson sphere would be much smaller and harder to detect. If intelligent aliens are out there, it may be a while yet before our scopes are powerful enough that we're able spot them from Earth. [arXiv via MIT Technology Review]
Top image via Slawek Wojtowicz
A small footnote: The researchers estimate that a Dyson sphere surrounding a white dwarf would be roughly 10 ^6 kilometers in radius. As pointed out by an astute commentator, this puts the newly proposed Dyson sphere within an order of magnitude of the one featured in Star Trek: The Next Generation. It may be new to science, but it seems Star Trek figured this all out loooong ago.
Contact the author at maddie.stone@gizmodo.com or follow her on Twitter.
As an exercise, how big would the Dyson sphere around this star be, and what would be its surface gravity?
Sirius B
With a mass nearly equal to the Sun's, Sirius B is one of the more massive white dwarfs known (0.98 M☉[102]); it is almost double the 0.5–0.6 M☉ average. Yet that same mass is packed into a volume roughly equal to the Earth's.[102] The current surface temperature is 25,200 K.[7] However, because there is no internal heat source, Sirius B will steadily cool as the remaining heat is radiated into space over a period of more than two billion years.[103]
A white dwarf forms only after the star has evolved from the main sequence and then passed through a red-giant stage. This occurred when Sirius B was less than half its current age, around 120 million years ago. The original star had an estimated 5 M☉[7] and was a B-type star (roughly B4–5)[104][105] when it still was on the main sequence. While it passed through the red giant stage, Sirius B may have enriched the metallicity of its companion.
This star is primarily composed of a carbon–oxygen mixture that was generated by helium fusion in the progenitor star.[7] This is overlaid by an envelope of lighter elements, with the materials segregated by mass because of the high surface gravity.[106] Hence the outer atmosphere of Sirius B is now almost pure hydrogen—the element with the lowest mass—and no other elements are seen in its spectrum.[107]